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information_for_astronomers:rx:s60mm [2013/03/12 14:09]
127.0.0.1 external edit
information_for_astronomers:rx:s60mm [2023/12/18 22:10] (current)
akraus
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 ^ Frequency [GHz] ^ Channel ^ Polarisation ^ Tcal [K] ^ Tsys [K] ^ Sensitivity [K/Jy] ^ SEFD [Jy] ^ Aperture Eff. [%] ^ TMB/S [K/Jy] ^ Main Beam Eff. [%] ^ FWHM [arcsec] ^ Last update ^ ^ Frequency [GHz] ^ Channel ^ Polarisation ^ Tcal [K] ^ Tsys [K] ^ Sensitivity [K/Jy] ^ SEFD [Jy] ^ Aperture Eff. [%] ^ TMB/S [K/Jy] ^ Main Beam Eff. [%] ^ FWHM [arcsec] ^ Last update ^
-|4.850 |A / B | LCP / RCP |1.8 |27 |1.55 |18 |53 |2.4 |63 |146 |June 2008|+|4.850 |A / B |LCP / RCP |1.8 |27 |1.55 |18 |53 |2.4 |63 |146 |June 2008|
  
 ^ normalized Gain curve (G = A0 + A1·Elv + A2·Elv2)^^^ Observed in ^ confirmed ^ ^ normalized Gain curve (G = A0 + A1·Elv + A2·Elv2)^^^ Observed in ^ confirmed ^
-|A0 = 0.97323|A1 = 1.2702E-3|A2 = -1.5059E-5|May 2004|  | +|A0 = 0.9870|A1 = 8.692E-4|A2 = -1.453E-5|Aug 2023|  |
-|A0 = 0.995|A1 = 5.2022E-4|A2 = -1.27874e-05|Feb 2008|  |+
  
 **Comments:​** **Comments:​**
   * The values for LCP and RCP do not differ significantly.   * The values for LCP and RCP do not differ significantly.
-  * The new gain curve (Feb 2007) was corrected for opacity. +  * The opacity ​is usually very smallTypical ​zenith tau values are < 0.01.
-  * If no other information about the opacity is available a typical ​zenith tau value of about 0.016 should do a good job+
  
 ==== Version description for OBSINP ==== ==== Version description for OBSINP ====
Line 62: Line 60:
 |  16  |   VLBA |   ​cross ​  | Horn 1, sin AB  | |  16  |   VLBA |   ​cross ​  | Horn 1, sin AB  |
  
 +==== Spectroscopy modes and resolution ====
 +^   BW ^ nchan ^    nu ^     Df ^     Dv ^     dv ^
 +^  MHz ^       ​^ ​  MHz ^    kHz ^   km/s ^   km/s ^
 +|  100 | 32768 |  4600 |    3.1 |  0.199 |  0.231 |
 +|  100 | 32768 |  4700 |    3.1 |  0.195 |  0.226 |
 +|  100 | 32768 |  4800 |    3.1 |  0.191 |  0.221 |
 +|  100 | 32768 |  4900 |    3.1 |  0.187 |  0.217 |
 +|  100 | 32768 |  5000 |    3.1 |  0.183 |  0.212 |
 +|  100 | 32768 |  5100 |    3.1 |  0.179 |  0.208 |
 +|  500 | 32768 |  4600 |   15.3 |  0.994 |  1.154 |
 +|  500 | 32768 |  4700 |   15.3 |  0.973 |  1.129 |
 +|  500 | 32768 |  4800 |   15.3 |  0.953 |  1.105 |
 +|  500 | 32768 |  4900 |   15.3 |  0.934 |  1.083 |
 +|  500 | 32768 |  5000 |   15.3 |  0.915 |  1.061 |
 +|  500 | 32768 |  5100 |   15.3 |  0.897 |  1.040 |
  
 +BW    ... band width\\
 +nchan ... number of spectral channels\\
 +nu    ... center frequency\\
 +Df    ... Channel separation (in frequency)\\
 +Dv    ... Channel separation (in velocity)\\
 +dv    ... Velocity resolution (dv=1.16*Dv)
  
-==== Tcal and Tsys measurements ==== 
-{{:​information_for_astronomers:​rx:​s60mm-xffts-tcal.png?​900|Tcal}} 
  
-{{:​information_for_astronomers:​rx:​s60mm-xffts-tsys.png?900|Tsys}}+==== Tcal and Tsys measurements ==== 
 +{{:​information_for_astronomers:​rx:​s60mmb_tcal_from_specpointing_using_tau_spec.png?675 |}} 
 +{{:​information_for_astronomers:​rx:​s60mmb_tsys0_from_specpointing_using_tau_spec.png?​675 |}} 
 +{{:​information_for_astronomers:​rx:​s60mmb_tau_from_specpointing_using_tau_spec.png?​675 |}} 
 +{{:​information_for_astronomers:​rx:​s60mmb_hpbw_from_specpointing.png?​675 ​|}}
  
-{{:​information_for_astronomers:​rx:​s60mm-xffts-trms.png?​900|Trms}} 
  
  
information_for_astronomers/rx/s60mm.1363093752.txt.gz · Last modified: 2013/09/30 13:52 (external edit)